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1746 Brouwer

From Wikipedia, the free encyclopedia
Hilda asteroid

1746 Brouwer
Shape model ofBrouwer from itslightcurve
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date14 September 1963
Designations
(1746) Brouwer
Named after
Dirk Brouwer
(astronomer)[2]
1963 RF · 1940 WE
1947 QA
main-belt · Hilda[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc76.33 yr (27,878 days)
Aphelion4.7671AU
Perihelion3.1284 AU
3.9478 AU
Eccentricity0.2076
7.84yr (2,865 days)
292.05°
0° 7m 32.52s / day
Inclination8.3676°
321.96°
47.580°
Jupiter MOID0.8580 AU
TJupiter3.0040
Physical characteristics
Dimensions61.50±1.80 km[4]
62.523±0.492[5]
64.25±4.9 km(IRAS:2)[3][6]
19.7255±0.0005h[7]
19.8 h[8]
19.88±0.05 h[a]
0.0448±0.008(IRAS:2)[3][6]
0.048±0.006[5]
0.051±0.003[4]
Tholen =D[1] · D[3][5]
B–V = 0.721[1]
U–B = 0.227[1]
9.78±0.30[9] · 9.95(IRAS:2)[6] · 9.95[3][4]

1746 Brouwer (prov. designation:1963 RF) is aHilda asteroid from the outermost region of theasteroid belt, approximately 64 kilometers in diameter. It was discovered on 14 September 1963, byIU'sIndiana Asteroid Program atGoethe Link Observatory near Brooklyn, Indiana, United States.[10] It was named after astronomerDirk Brouwer.[2]

Classification and orbit

[edit]

Brouwer is a member of theHilda family (001), an asteroid family within the dynamicalHilda group, a large group that orbits inresonance with the gas giant Jupiter and are thought to originate from theKuiper belt.Brouwer orbits the Sun at a distance of 3.1–4.8 AU once every 7 years and 10 months (2,865 days). Its orbit has aneccentricity of 0.21 and aninclination of 8° with respect to theecliptic.[1]

It was first identified as1940 WE atTurku Observatory in 1940, extending the body'sobservation arc by 23 years prior to its official discovery observation.[10]

Physical characteristics

[edit]

In theTholen classification,Brouwer is characterized as a dark and reddishD-type asteroid.[1]

Rotation period

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Several rotationallightcurves ofBrouwer gave arotation period between 19.72 and 19.88 hours with a brightness variation of 0.21 and 0.35magnitude (U=n.a/2/n.a.).[7][8][a]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Brouwer measures between 61.50 and 64.25 kilometers in diameter, and its surface has analbedo between 0.045 and 0.051.[4][5][6]

TheCollaborative Asteroid Lightcurve Link agrees with IRAS, that is an albedo of 0.045 and a diameter of 64.25 kilometers with anabsolute magnitude of 9.95.[3]

Naming

[edit]

Thisminor planet was named in honor of Dutch–American astronomerDirk Brouwer (1902–1966). Originally atLeiden University and specialized incelestial mechanics, he became director of theYale University Observatory and was the president ofIAU's commission 20,Positions & Motions of Minor Planets, Comets & Satellites, from 1948 to 1955.[2] The officialnaming citation was published by theMinor Planet Center on 15 July 1968 (M.P.C. 2883).[11]

Notes

[edit]
  1. ^abSlyusarev (2012) web: rotation period19.88±0.05 hours with a brightness amplitude of0.21. Summary figures atAsteroid Lightcurve Database for (1746) Brouwer

References

[edit]
  1. ^abcdefg"JPL Small-Body Database Browser: 1746 Brouwer (1963 RF)" (2017-03-28 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 5 August 2020. Retrieved7 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1746) Brouwer".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 139.doi:10.1007/978-3-540-29925-7_1747.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1746) Brouwer". Asteroid Lightcurve Database (LCDB). Retrieved20 December 2016.
  4. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  5. ^abcdGrav, T.; Mainzer, A. K.; Bauer, J.; Masiero, J.; Spahr, T.; McMillan, R. S.; et al. (January 2012)."WISE/NEOWISE Observations of the Hilda Population: Preliminary Results".The Astrophysical Journal.744 (2): 15.arXiv:1110.0283.Bibcode:2012ApJ...744..197G.doi:10.1088/0004-637X/744/2/197.S2CID 44000310. Retrieved20 December 2016.
  6. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.12.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  7. ^abHanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016)."New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: 24.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.S2CID 119112278. Retrieved20 December 2016.
  8. ^abDahlgren, M.; Lahulla, J. F.; Lagerkvist, C.-I.; Lagerros, J.; Mottola, S.; Erikson, A.; et al. (June 1998)."A Study of Hilda Asteroids. V. Lightcurves of 47 Hilda Asteroids".Icarus.133 (2):247–285.Bibcode:1998Icar..133..247D.doi:10.1006/icar.1998.5919. Retrieved20 December 2016.
  9. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved20 December 2016.
  10. ^ab"1746 Brouwer (1963 RF)".Minor Planet Center. Retrieved20 December 2016.
  11. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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